The Bateman equation gives a centralized expression for determining the number of panicles of the n^m radioactive member of a generalized dosed decay chain at any time. t. The equation assumes that initially there are only N_10 particles of the parent species prevent the equation is given by. with the provision that lambda_n - lambda_n = 1.0 The Voyager 1 and 2 space probes were launched by NASA on September 5. 1977 and August 20. 1977. respectively. The probes were built with 3 Multiheaded-Watt radioisotope thermoelectric generators (MHW RTGs) and powered with 24 pressed plutonium (_94Pu^238) oxide spheres. Using the expanded _94Pu^238 decay chain shown below, develop a computer program to calculate the number ratio. N/N_10 from Eq. (1) for all members of the decay chain as a function of time. Use the half-life values in the figure to determine the decay constant for each member. Print the number ratios for all members for the following times; 10, 20, 30, 40 years. The Bateman equation gives a centralized expression for determining the number of panicles of the n^m radioactive member of a generalized dosed decay chain at any time. t. The equation assumes that initially there are only N_10 particles of the parent species prevent the equation is given by. with the provision that lambda_n - lambda_n = 1.0 The Voyager 1 and 2 space probes were launched by NASA on September 5. 1977 and August 20. 1977. respectively. The probes were built with 3 Multiheaded-Watt radioisotope thermoelectric generators (MHW RTGs) and powered with 24 pressed plutonium (_94Pu^238) oxide spheres. Using the expanded _94Pu^238 decay chain shown below, develop a computer program to calculate the number ratio. N/N_10 from Eq. (1) for all members of the decay chain as a function of time. Use the half-life values in the figure to determine the decay constant for each member. Print the number ratios for all members for the following times; 10, 20, 30, 40 years